大宇宙中的科学

M. Srednicki, J. Hartle
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引用次数: 16

摘要

作为宇宙的观察者,我们是宇宙中的量子物理系统。如果宇宙在空间和/或时间上非常大,那么我们所依据的预测数据在时空的其他位置被复制的可能性就变得非常大。数据中未指定的这些位置的物理条件可能会有所不同。因此,对我们未来观测的预测需要一个假设的概率分布(静电照相分布),以确定我们在可能分布中的位置。只有把基本理论和静电照相分布结合起来,才能通过进一步的观察加以预测和检验。
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Science in a Very Large Universe
As observers of the universe we are quantum physical systems within it. If the universe is very large in space and/or time, the probability becomes significant that the data on which we base predictions is replicated at other locations in spacetime. The physical conditions at these locations that are not specified by the data may differ. Predictions of our future observations therefore require an assumed probability distribution (the xerographic distribution) for our location among the possible ones. It is the combination of basic theory plus the xerographic distribution that can be predictive and testable by further observations.
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